Limits on dark matter annihilation in the sun using the ANTARES neutrino telescope
A search for muon neutrinos originating from dark matter annihilations in the Sun is performed using the data recorded by the ANTARES neutrino telescope from 2007 to 2012. In order to obtain the best possible sensitivities to dark matter signals, an optimisation of the event selection criteria is pe...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Adrián-Martínez, S. [verfasserIn] |
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| Format: |
E-Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
2016transfer abstract |
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| Schlagwörter: |
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| Umfang: |
6 |
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| Übergeordnetes Werk: |
Enthalten in: Applying the Go/NoGo processing schema to a visual oddball task in older adults - Steiner, Genevieve Z. ELSEVIER, 2016, Amsterdam |
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| Übergeordnetes Werk: |
volume:759 ; year:2016 ; day:10 ; month:08 ; pages:69-74 ; extent:6 |
| Links: |
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| DOI / URN: |
10.1016/j.physletb.2016.05.019 |
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| Katalog-ID: |
ELV01408001X |
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| 245 | 1 | 0 | |a Limits on dark matter annihilation in the sun using the ANTARES neutrino telescope |
| 264 | 1 | |c 2016transfer abstract | |
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| 520 | |a A search for muon neutrinos originating from dark matter annihilations in the Sun is performed using the data recorded by the ANTARES neutrino telescope from 2007 to 2012. In order to obtain the best possible sensitivities to dark matter signals, an optimisation of the event selection criteria is performed taking into account the background of atmospheric muons, atmospheric neutrinos and the energy spectra of the expected neutrino signals. No significant excess over the background is observed and 90 % C.L. upper limits on the neutrino flux, the spin-dependent and spin-independent WIMP-nucleon cross-sections are derived for WIMP masses ranging from 50 GeV to 5 TeV for the annihilation channels WIMP + WIMP → b b ¯ , W + W − and τ + τ − . | ||
| 520 | |a A search for muon neutrinos originating from dark matter annihilations in the Sun is performed using the data recorded by the ANTARES neutrino telescope from 2007 to 2012. In order to obtain the best possible sensitivities to dark matter signals, an optimisation of the event selection criteria is performed taking into account the background of atmospheric muons, atmospheric neutrinos and the energy spectra of the expected neutrino signals. No significant excess over the background is observed and 90 % C.L. upper limits on the neutrino flux, the spin-dependent and spin-independent WIMP-nucleon cross-sections are derived for WIMP masses ranging from 50 GeV to 5 TeV for the annihilation channels WIMP + WIMP → b b ¯ , W + W − and τ + τ − . | ||
| 650 | 7 | |a Dark matter |2 Elsevier | |
| 650 | 7 | |a Neutrino telescope |2 Elsevier | |
| 650 | 7 | |a Indirect detection |2 Elsevier | |
| 650 | 7 | |a WIMP |2 Elsevier | |
| 650 | 7 | |a Neutralino |2 Elsevier | |
| 650 | 7 | |a Sun |2 Elsevier | |
| 700 | 1 | |a Albert, A. |4 oth | |
| 700 | 1 | |a André, M. |4 oth | |
| 700 | 1 | |a Anton, G. |4 oth | |
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10.1016/j.physletb.2016.05.019 doi GBV00000000000250A.pica (DE-627)ELV01408001X (ELSEVIER)S0370-2693(16)30166-6 DE-627 ger DE-627 rakwb eng 530 DE-600 610 VZ 77.50 bkl Adrián-Martínez, S. verfasserin aut Limits on dark matter annihilation in the sun using the ANTARES neutrino telescope 2016transfer abstract 6 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier A search for muon neutrinos originating from dark matter annihilations in the Sun is performed using the data recorded by the ANTARES neutrino telescope from 2007 to 2012. In order to obtain the best possible sensitivities to dark matter signals, an optimisation of the event selection criteria is performed taking into account the background of atmospheric muons, atmospheric neutrinos and the energy spectra of the expected neutrino signals. No significant excess over the background is observed and 90 % C.L. upper limits on the neutrino flux, the spin-dependent and spin-independent WIMP-nucleon cross-sections are derived for WIMP masses ranging from 50 GeV to 5 TeV for the annihilation channels WIMP + WIMP → b b ¯ , W + W − and τ + τ − . A search for muon neutrinos originating from dark matter annihilations in the Sun is performed using the data recorded by the ANTARES neutrino telescope from 2007 to 2012. In order to obtain the best possible sensitivities to dark matter signals, an optimisation of the event selection criteria is performed taking into account the background of atmospheric muons, atmospheric neutrinos and the energy spectra of the expected neutrino signals. No significant excess over the background is observed and 90 % C.L. upper limits on the neutrino flux, the spin-dependent and spin-independent WIMP-nucleon cross-sections are derived for WIMP masses ranging from 50 GeV to 5 TeV for the annihilation channels WIMP + WIMP → b b ¯ , W + W − and τ + τ − . Dark matter Elsevier Neutrino telescope Elsevier Indirect detection Elsevier WIMP Elsevier Neutralino Elsevier Sun Elsevier Albert, A. oth André, M. oth Anton, G. oth Ardid, M. oth Aubert, J.-J. oth Avgitas, T. oth Baret, B. oth Barrios-Martí, J. oth Basa, S. oth Bertin, V. oth Biagi, S. oth Bormuth, R. oth Bouwhuis, M.C. oth Bruijn, R. oth Brunner, J. oth Busto, J. oth Capone, A. oth Caramete, L. oth Carr, J. oth Celli, S. oth Chiarusi, T. oth Circella, M. oth Coleiro, A. oth Coniglione, R. oth Costantini, H. oth Coyle, P. oth Creusot, A. oth Deschamps, A. oth De Bonis, G. oth Distefano, C. oth Donzaud, C. oth Dornic, D. oth Drouhin, D. oth Eberl, T. oth El Bojaddaini, I. oth Elsässer, D. oth Enzenhöfer, A. oth Fehn, K. oth Felis, I. oth Fusco, L.A. oth Galatà, S. oth Gay, P. oth Geißelsöder, S. oth Geyer, K. oth Giordano, V. oth Gleixner, A. oth Glotin, H. oth Gracia-Ruiz, R. oth Graf, K. oth Hallmann, S. oth van Haren, H. oth Heijboer, A.J. oth Hello, Y. oth Hernández-Rey, J.J. oth Hößl, J. oth Hofestädt, J. oth Hugon, C. oth Illuminati, G. oth James, C.W. oth de Jong, M. oth Jongen, M. oth Kadler, M. oth Kalekin, O. oth Katz, U. oth Kießling, D. oth Kouchner, A. oth Kreter, M. oth Kreykenbohm, I. oth Kulikovskiy, V. oth Lachaud, C. oth Lahmann, R. oth Lefèvre, D. oth Leonora, E. oth Loucatos, S. oth Marcelin, M. oth Margiotta, A. oth Marinelli, A. oth Martínez-Mora, J.A. oth Mathieu, A. oth Melis, K. oth Michael, T. oth Migliozzi, P. oth Moussa, A. oth Mueller, C. oth Nezri, E. oth Păvălaş, G.E. oth Pellegrino, C. oth Perrina, C. oth Piattelli, P. oth Popa, V. oth Pradier, T. oth Racca, C. oth Riccobene, G. oth Roensch, K. oth Saldaña, M. oth Samtleben, D.F.E. oth Sánchez-Losa, A. oth Sanguineti, M. oth Sapienza, P. oth Schnabel, J. oth Schüssler, F. oth Seitz, T. oth Sieger, C. oth Spurio, M. oth Stolarczyk, Th. oth Taiuti, M. oth Tönnis, C. oth Trovato, A. oth Tselengidou, M. oth Turpin, D. oth Vallage, B. oth Vallée, C. oth Van Elewyck, V. oth Vivolo, D. oth Wagner, S. oth Wilms, J. oth Zornoza, J.D. oth Zúñiga, J. oth Enthalten in North-Holland Publ Steiner, Genevieve Z. ELSEVIER Applying the Go/NoGo processing schema to a visual oddball task in older adults 2016 Amsterdam (DE-627)ELV000151122 volume:759 year:2016 day:10 month:08 pages:69-74 extent:6 https://doi.org/10.1016/j.physletb.2016.05.019 Volltext GBV_USEFLAG_U GBV_ELV SYSFLAG_U SSG-OLC-PHA 77.50 Psychophysiologie VZ AR 759 2016 10 0810 69-74 6 |
| spelling |
10.1016/j.physletb.2016.05.019 doi GBV00000000000250A.pica (DE-627)ELV01408001X (ELSEVIER)S0370-2693(16)30166-6 DE-627 ger DE-627 rakwb eng 530 DE-600 610 VZ 77.50 bkl Adrián-Martínez, S. verfasserin aut Limits on dark matter annihilation in the sun using the ANTARES neutrino telescope 2016transfer abstract 6 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier A search for muon neutrinos originating from dark matter annihilations in the Sun is performed using the data recorded by the ANTARES neutrino telescope from 2007 to 2012. In order to obtain the best possible sensitivities to dark matter signals, an optimisation of the event selection criteria is performed taking into account the background of atmospheric muons, atmospheric neutrinos and the energy spectra of the expected neutrino signals. No significant excess over the background is observed and 90 % C.L. upper limits on the neutrino flux, the spin-dependent and spin-independent WIMP-nucleon cross-sections are derived for WIMP masses ranging from 50 GeV to 5 TeV for the annihilation channels WIMP + WIMP → b b ¯ , W + W − and τ + τ − . A search for muon neutrinos originating from dark matter annihilations in the Sun is performed using the data recorded by the ANTARES neutrino telescope from 2007 to 2012. In order to obtain the best possible sensitivities to dark matter signals, an optimisation of the event selection criteria is performed taking into account the background of atmospheric muons, atmospheric neutrinos and the energy spectra of the expected neutrino signals. No significant excess over the background is observed and 90 % C.L. upper limits on the neutrino flux, the spin-dependent and spin-independent WIMP-nucleon cross-sections are derived for WIMP masses ranging from 50 GeV to 5 TeV for the annihilation channels WIMP + WIMP → b b ¯ , W + W − and τ + τ − . Dark matter Elsevier Neutrino telescope Elsevier Indirect detection Elsevier WIMP Elsevier Neutralino Elsevier Sun Elsevier Albert, A. oth André, M. oth Anton, G. oth Ardid, M. oth Aubert, J.-J. oth Avgitas, T. oth Baret, B. oth Barrios-Martí, J. oth Basa, S. oth Bertin, V. oth Biagi, S. oth Bormuth, R. oth Bouwhuis, M.C. oth Bruijn, R. oth Brunner, J. oth Busto, J. oth Capone, A. oth Caramete, L. oth Carr, J. oth Celli, S. oth Chiarusi, T. oth Circella, M. oth Coleiro, A. oth Coniglione, R. oth Costantini, H. oth Coyle, P. oth Creusot, A. oth Deschamps, A. oth De Bonis, G. oth Distefano, C. oth Donzaud, C. oth Dornic, D. oth Drouhin, D. oth Eberl, T. oth El Bojaddaini, I. oth Elsässer, D. oth Enzenhöfer, A. oth Fehn, K. oth Felis, I. oth Fusco, L.A. oth Galatà, S. oth Gay, P. oth Geißelsöder, S. oth Geyer, K. oth Giordano, V. oth Gleixner, A. oth Glotin, H. oth Gracia-Ruiz, R. oth Graf, K. oth Hallmann, S. oth van Haren, H. oth Heijboer, A.J. oth Hello, Y. oth Hernández-Rey, J.J. oth Hößl, J. oth Hofestädt, J. oth Hugon, C. oth Illuminati, G. oth James, C.W. oth de Jong, M. oth Jongen, M. oth Kadler, M. oth Kalekin, O. oth Katz, U. oth Kießling, D. oth Kouchner, A. oth Kreter, M. oth Kreykenbohm, I. oth Kulikovskiy, V. oth Lachaud, C. oth Lahmann, R. oth Lefèvre, D. oth Leonora, E. oth Loucatos, S. oth Marcelin, M. oth Margiotta, A. oth Marinelli, A. oth Martínez-Mora, J.A. oth Mathieu, A. oth Melis, K. oth Michael, T. oth Migliozzi, P. oth Moussa, A. oth Mueller, C. oth Nezri, E. oth Păvălaş, G.E. oth Pellegrino, C. oth Perrina, C. oth Piattelli, P. oth Popa, V. oth Pradier, T. oth Racca, C. oth Riccobene, G. oth Roensch, K. oth Saldaña, M. oth Samtleben, D.F.E. oth Sánchez-Losa, A. oth Sanguineti, M. oth Sapienza, P. oth Schnabel, J. oth Schüssler, F. oth Seitz, T. oth Sieger, C. oth Spurio, M. oth Stolarczyk, Th. oth Taiuti, M. oth Tönnis, C. oth Trovato, A. oth Tselengidou, M. oth Turpin, D. oth Vallage, B. oth Vallée, C. oth Van Elewyck, V. oth Vivolo, D. oth Wagner, S. oth Wilms, J. oth Zornoza, J.D. oth Zúñiga, J. oth Enthalten in North-Holland Publ Steiner, Genevieve Z. ELSEVIER Applying the Go/NoGo processing schema to a visual oddball task in older adults 2016 Amsterdam (DE-627)ELV000151122 volume:759 year:2016 day:10 month:08 pages:69-74 extent:6 https://doi.org/10.1016/j.physletb.2016.05.019 Volltext GBV_USEFLAG_U GBV_ELV SYSFLAG_U SSG-OLC-PHA 77.50 Psychophysiologie VZ AR 759 2016 10 0810 69-74 6 |
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10.1016/j.physletb.2016.05.019 doi GBV00000000000250A.pica (DE-627)ELV01408001X (ELSEVIER)S0370-2693(16)30166-6 DE-627 ger DE-627 rakwb eng 530 DE-600 610 VZ 77.50 bkl Adrián-Martínez, S. verfasserin aut Limits on dark matter annihilation in the sun using the ANTARES neutrino telescope 2016transfer abstract 6 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier A search for muon neutrinos originating from dark matter annihilations in the Sun is performed using the data recorded by the ANTARES neutrino telescope from 2007 to 2012. In order to obtain the best possible sensitivities to dark matter signals, an optimisation of the event selection criteria is performed taking into account the background of atmospheric muons, atmospheric neutrinos and the energy spectra of the expected neutrino signals. No significant excess over the background is observed and 90 % C.L. upper limits on the neutrino flux, the spin-dependent and spin-independent WIMP-nucleon cross-sections are derived for WIMP masses ranging from 50 GeV to 5 TeV for the annihilation channels WIMP + WIMP → b b ¯ , W + W − and τ + τ − . A search for muon neutrinos originating from dark matter annihilations in the Sun is performed using the data recorded by the ANTARES neutrino telescope from 2007 to 2012. In order to obtain the best possible sensitivities to dark matter signals, an optimisation of the event selection criteria is performed taking into account the background of atmospheric muons, atmospheric neutrinos and the energy spectra of the expected neutrino signals. No significant excess over the background is observed and 90 % C.L. upper limits on the neutrino flux, the spin-dependent and spin-independent WIMP-nucleon cross-sections are derived for WIMP masses ranging from 50 GeV to 5 TeV for the annihilation channels WIMP + WIMP → b b ¯ , W + W − and τ + τ − . Dark matter Elsevier Neutrino telescope Elsevier Indirect detection Elsevier WIMP Elsevier Neutralino Elsevier Sun Elsevier Albert, A. oth André, M. oth Anton, G. oth Ardid, M. oth Aubert, J.-J. oth Avgitas, T. oth Baret, B. oth Barrios-Martí, J. oth Basa, S. oth Bertin, V. oth Biagi, S. oth Bormuth, R. oth Bouwhuis, M.C. oth Bruijn, R. oth Brunner, J. oth Busto, J. oth Capone, A. oth Caramete, L. oth Carr, J. oth Celli, S. oth Chiarusi, T. oth Circella, M. oth Coleiro, A. oth Coniglione, R. oth Costantini, H. oth Coyle, P. oth Creusot, A. oth Deschamps, A. oth De Bonis, G. oth Distefano, C. oth Donzaud, C. oth Dornic, D. oth Drouhin, D. oth Eberl, T. oth El Bojaddaini, I. oth Elsässer, D. oth Enzenhöfer, A. oth Fehn, K. oth Felis, I. oth Fusco, L.A. oth Galatà, S. oth Gay, P. oth Geißelsöder, S. oth Geyer, K. oth Giordano, V. oth Gleixner, A. oth Glotin, H. oth Gracia-Ruiz, R. oth Graf, K. oth Hallmann, S. oth van Haren, H. oth Heijboer, A.J. oth Hello, Y. oth Hernández-Rey, J.J. oth Hößl, J. oth Hofestädt, J. oth Hugon, C. oth Illuminati, G. oth James, C.W. oth de Jong, M. oth Jongen, M. oth Kadler, M. oth Kalekin, O. oth Katz, U. oth Kießling, D. oth Kouchner, A. oth Kreter, M. oth Kreykenbohm, I. oth Kulikovskiy, V. oth Lachaud, C. oth Lahmann, R. oth Lefèvre, D. oth Leonora, E. oth Loucatos, S. oth Marcelin, M. oth Margiotta, A. oth Marinelli, A. oth Martínez-Mora, J.A. oth Mathieu, A. oth Melis, K. oth Michael, T. oth Migliozzi, P. oth Moussa, A. oth Mueller, C. oth Nezri, E. oth Păvălaş, G.E. oth Pellegrino, C. oth Perrina, C. oth Piattelli, P. oth Popa, V. oth Pradier, T. oth Racca, C. oth Riccobene, G. oth Roensch, K. oth Saldaña, M. oth Samtleben, D.F.E. oth Sánchez-Losa, A. oth Sanguineti, M. oth Sapienza, P. oth Schnabel, J. oth Schüssler, F. oth Seitz, T. oth Sieger, C. oth Spurio, M. oth Stolarczyk, Th. oth Taiuti, M. oth Tönnis, C. oth Trovato, A. oth Tselengidou, M. oth Turpin, D. oth Vallage, B. oth Vallée, C. oth Van Elewyck, V. oth Vivolo, D. oth Wagner, S. oth Wilms, J. oth Zornoza, J.D. oth Zúñiga, J. oth Enthalten in North-Holland Publ Steiner, Genevieve Z. ELSEVIER Applying the Go/NoGo processing schema to a visual oddball task in older adults 2016 Amsterdam (DE-627)ELV000151122 volume:759 year:2016 day:10 month:08 pages:69-74 extent:6 https://doi.org/10.1016/j.physletb.2016.05.019 Volltext GBV_USEFLAG_U GBV_ELV SYSFLAG_U SSG-OLC-PHA 77.50 Psychophysiologie VZ AR 759 2016 10 0810 69-74 6 |
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10.1016/j.physletb.2016.05.019 doi GBV00000000000250A.pica (DE-627)ELV01408001X (ELSEVIER)S0370-2693(16)30166-6 DE-627 ger DE-627 rakwb eng 530 DE-600 610 VZ 77.50 bkl Adrián-Martínez, S. verfasserin aut Limits on dark matter annihilation in the sun using the ANTARES neutrino telescope 2016transfer abstract 6 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier A search for muon neutrinos originating from dark matter annihilations in the Sun is performed using the data recorded by the ANTARES neutrino telescope from 2007 to 2012. In order to obtain the best possible sensitivities to dark matter signals, an optimisation of the event selection criteria is performed taking into account the background of atmospheric muons, atmospheric neutrinos and the energy spectra of the expected neutrino signals. No significant excess over the background is observed and 90 % C.L. upper limits on the neutrino flux, the spin-dependent and spin-independent WIMP-nucleon cross-sections are derived for WIMP masses ranging from 50 GeV to 5 TeV for the annihilation channels WIMP + WIMP → b b ¯ , W + W − and τ + τ − . A search for muon neutrinos originating from dark matter annihilations in the Sun is performed using the data recorded by the ANTARES neutrino telescope from 2007 to 2012. In order to obtain the best possible sensitivities to dark matter signals, an optimisation of the event selection criteria is performed taking into account the background of atmospheric muons, atmospheric neutrinos and the energy spectra of the expected neutrino signals. No significant excess over the background is observed and 90 % C.L. upper limits on the neutrino flux, the spin-dependent and spin-independent WIMP-nucleon cross-sections are derived for WIMP masses ranging from 50 GeV to 5 TeV for the annihilation channels WIMP + WIMP → b b ¯ , W + W − and τ + τ − . Dark matter Elsevier Neutrino telescope Elsevier Indirect detection Elsevier WIMP Elsevier Neutralino Elsevier Sun Elsevier Albert, A. oth André, M. oth Anton, G. oth Ardid, M. oth Aubert, J.-J. oth Avgitas, T. oth Baret, B. oth Barrios-Martí, J. oth Basa, S. oth Bertin, V. oth Biagi, S. oth Bormuth, R. oth Bouwhuis, M.C. oth Bruijn, R. oth Brunner, J. oth Busto, J. oth Capone, A. oth Caramete, L. oth Carr, J. oth Celli, S. oth Chiarusi, T. oth Circella, M. oth Coleiro, A. oth Coniglione, R. oth Costantini, H. oth Coyle, P. oth Creusot, A. oth Deschamps, A. oth De Bonis, G. oth Distefano, C. oth Donzaud, C. oth Dornic, D. oth Drouhin, D. oth Eberl, T. oth El Bojaddaini, I. oth Elsässer, D. oth Enzenhöfer, A. oth Fehn, K. oth Felis, I. oth Fusco, L.A. oth Galatà, S. oth Gay, P. oth Geißelsöder, S. oth Geyer, K. oth Giordano, V. oth Gleixner, A. oth Glotin, H. oth Gracia-Ruiz, R. oth Graf, K. oth Hallmann, S. oth van Haren, H. oth Heijboer, A.J. oth Hello, Y. oth Hernández-Rey, J.J. oth Hößl, J. oth Hofestädt, J. oth Hugon, C. oth Illuminati, G. oth James, C.W. oth de Jong, M. oth Jongen, M. oth Kadler, M. oth Kalekin, O. oth Katz, U. oth Kießling, D. oth Kouchner, A. oth Kreter, M. oth Kreykenbohm, I. oth Kulikovskiy, V. oth Lachaud, C. oth Lahmann, R. oth Lefèvre, D. oth Leonora, E. oth Loucatos, S. oth Marcelin, M. oth Margiotta, A. oth Marinelli, A. oth Martínez-Mora, J.A. oth Mathieu, A. oth Melis, K. oth Michael, T. oth Migliozzi, P. oth Moussa, A. oth Mueller, C. oth Nezri, E. oth Păvălaş, G.E. oth Pellegrino, C. oth Perrina, C. oth Piattelli, P. oth Popa, V. oth Pradier, T. oth Racca, C. oth Riccobene, G. oth Roensch, K. oth Saldaña, M. oth Samtleben, D.F.E. oth Sánchez-Losa, A. oth Sanguineti, M. oth Sapienza, P. oth Schnabel, J. oth Schüssler, F. oth Seitz, T. oth Sieger, C. oth Spurio, M. oth Stolarczyk, Th. oth Taiuti, M. oth Tönnis, C. oth Trovato, A. oth Tselengidou, M. oth Turpin, D. oth Vallage, B. oth Vallée, C. oth Van Elewyck, V. oth Vivolo, D. oth Wagner, S. oth Wilms, J. oth Zornoza, J.D. oth Zúñiga, J. oth Enthalten in North-Holland Publ Steiner, Genevieve Z. ELSEVIER Applying the Go/NoGo processing schema to a visual oddball task in older adults 2016 Amsterdam (DE-627)ELV000151122 volume:759 year:2016 day:10 month:08 pages:69-74 extent:6 https://doi.org/10.1016/j.physletb.2016.05.019 Volltext GBV_USEFLAG_U GBV_ELV SYSFLAG_U SSG-OLC-PHA 77.50 Psychophysiologie VZ AR 759 2016 10 0810 69-74 6 |
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10.1016/j.physletb.2016.05.019 doi GBV00000000000250A.pica (DE-627)ELV01408001X (ELSEVIER)S0370-2693(16)30166-6 DE-627 ger DE-627 rakwb eng 530 DE-600 610 VZ 77.50 bkl Adrián-Martínez, S. verfasserin aut Limits on dark matter annihilation in the sun using the ANTARES neutrino telescope 2016transfer abstract 6 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier A search for muon neutrinos originating from dark matter annihilations in the Sun is performed using the data recorded by the ANTARES neutrino telescope from 2007 to 2012. In order to obtain the best possible sensitivities to dark matter signals, an optimisation of the event selection criteria is performed taking into account the background of atmospheric muons, atmospheric neutrinos and the energy spectra of the expected neutrino signals. No significant excess over the background is observed and 90 % C.L. upper limits on the neutrino flux, the spin-dependent and spin-independent WIMP-nucleon cross-sections are derived for WIMP masses ranging from 50 GeV to 5 TeV for the annihilation channels WIMP + WIMP → b b ¯ , W + W − and τ + τ − . A search for muon neutrinos originating from dark matter annihilations in the Sun is performed using the data recorded by the ANTARES neutrino telescope from 2007 to 2012. In order to obtain the best possible sensitivities to dark matter signals, an optimisation of the event selection criteria is performed taking into account the background of atmospheric muons, atmospheric neutrinos and the energy spectra of the expected neutrino signals. No significant excess over the background is observed and 90 % C.L. upper limits on the neutrino flux, the spin-dependent and spin-independent WIMP-nucleon cross-sections are derived for WIMP masses ranging from 50 GeV to 5 TeV for the annihilation channels WIMP + WIMP → b b ¯ , W + W − and τ + τ − . Dark matter Elsevier Neutrino telescope Elsevier Indirect detection Elsevier WIMP Elsevier Neutralino Elsevier Sun Elsevier Albert, A. oth André, M. oth Anton, G. oth Ardid, M. oth Aubert, J.-J. oth Avgitas, T. oth Baret, B. oth Barrios-Martí, J. oth Basa, S. oth Bertin, V. oth Biagi, S. oth Bormuth, R. oth Bouwhuis, M.C. oth Bruijn, R. oth Brunner, J. oth Busto, J. oth Capone, A. oth Caramete, L. oth Carr, J. oth Celli, S. oth Chiarusi, T. oth Circella, M. oth Coleiro, A. oth Coniglione, R. oth Costantini, H. oth Coyle, P. oth Creusot, A. oth Deschamps, A. oth De Bonis, G. oth Distefano, C. oth Donzaud, C. oth Dornic, D. oth Drouhin, D. oth Eberl, T. oth El Bojaddaini, I. oth Elsässer, D. oth Enzenhöfer, A. oth Fehn, K. oth Felis, I. oth Fusco, L.A. oth Galatà, S. oth Gay, P. oth Geißelsöder, S. oth Geyer, K. oth Giordano, V. oth Gleixner, A. oth Glotin, H. oth Gracia-Ruiz, R. oth Graf, K. oth Hallmann, S. oth van Haren, H. oth Heijboer, A.J. oth Hello, Y. oth Hernández-Rey, J.J. oth Hößl, J. oth Hofestädt, J. oth Hugon, C. oth Illuminati, G. oth James, C.W. oth de Jong, M. oth Jongen, M. oth Kadler, M. oth Kalekin, O. oth Katz, U. oth Kießling, D. oth Kouchner, A. oth Kreter, M. oth Kreykenbohm, I. oth Kulikovskiy, V. oth Lachaud, C. oth Lahmann, R. oth Lefèvre, D. oth Leonora, E. oth Loucatos, S. oth Marcelin, M. oth Margiotta, A. oth Marinelli, A. oth Martínez-Mora, J.A. oth Mathieu, A. oth Melis, K. oth Michael, T. oth Migliozzi, P. oth Moussa, A. oth Mueller, C. oth Nezri, E. oth Păvălaş, G.E. oth Pellegrino, C. oth Perrina, C. oth Piattelli, P. oth Popa, V. oth Pradier, T. oth Racca, C. oth Riccobene, G. oth Roensch, K. oth Saldaña, M. oth Samtleben, D.F.E. oth Sánchez-Losa, A. oth Sanguineti, M. oth Sapienza, P. oth Schnabel, J. oth Schüssler, F. oth Seitz, T. oth Sieger, C. oth Spurio, M. oth Stolarczyk, Th. oth Taiuti, M. oth Tönnis, C. oth Trovato, A. oth Tselengidou, M. oth Turpin, D. oth Vallage, B. oth Vallée, C. oth Van Elewyck, V. oth Vivolo, D. oth Wagner, S. oth Wilms, J. oth Zornoza, J.D. oth Zúñiga, J. oth Enthalten in North-Holland Publ Steiner, Genevieve Z. ELSEVIER Applying the Go/NoGo processing schema to a visual oddball task in older adults 2016 Amsterdam (DE-627)ELV000151122 volume:759 year:2016 day:10 month:08 pages:69-74 extent:6 https://doi.org/10.1016/j.physletb.2016.05.019 Volltext GBV_USEFLAG_U GBV_ELV SYSFLAG_U SSG-OLC-PHA 77.50 Psychophysiologie VZ AR 759 2016 10 0810 69-74 6 |
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In order to obtain the best possible sensitivities to dark matter signals, an optimisation of the event selection criteria is performed taking into account the background of atmospheric muons, atmospheric neutrinos and the energy spectra of the expected neutrino signals. No significant excess over the background is observed and 90 % C.L. upper limits on the neutrino flux, the spin-dependent and spin-independent WIMP-nucleon cross-sections are derived for WIMP masses ranging from 50 GeV to 5 TeV for the annihilation channels WIMP + WIMP → b b ¯ , W + W − and τ + τ − .</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">A search for muon neutrinos originating from dark matter annihilations in the Sun is performed using the data recorded by the ANTARES neutrino telescope from 2007 to 2012. 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| author |
Adrián-Martínez, S. |
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Adrián-Martínez, S. ddc 530 ddc 610 bkl 77.50 Elsevier Dark matter Elsevier Neutrino telescope Elsevier Indirect detection Elsevier WIMP Elsevier Neutralino Elsevier Sun Limits on dark matter annihilation in the sun using the ANTARES neutrino telescope |
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Adrián-Martínez, S. |
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530 - Physics 610 - Medicine & health |
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530 DE-600 610 VZ 77.50 bkl Limits on dark matter annihilation in the sun using the ANTARES neutrino telescope Dark matter Elsevier Neutrino telescope Elsevier Indirect detection Elsevier WIMP Elsevier Neutralino Elsevier Sun Elsevier |
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ddc 530 ddc 610 bkl 77.50 Elsevier Dark matter Elsevier Neutrino telescope Elsevier Indirect detection Elsevier WIMP Elsevier Neutralino Elsevier Sun |
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ddc 530 ddc 610 bkl 77.50 Elsevier Dark matter Elsevier Neutrino telescope Elsevier Indirect detection Elsevier WIMP Elsevier Neutralino Elsevier Sun |
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ddc 530 ddc 610 bkl 77.50 Elsevier Dark matter Elsevier Neutrino telescope Elsevier Indirect detection Elsevier WIMP Elsevier Neutralino Elsevier Sun |
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Elektronische Aufsätze Aufsätze Elektronische Ressource |
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Limits on dark matter annihilation in the sun using the ANTARES neutrino telescope |
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Limits on dark matter annihilation in the sun using the ANTARES neutrino telescope |
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Applying the Go/NoGo processing schema to a visual oddball task in older adults |
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limits on dark matter annihilation in the sun using the antares neutrino telescope |
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Limits on dark matter annihilation in the sun using the ANTARES neutrino telescope |
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A search for muon neutrinos originating from dark matter annihilations in the Sun is performed using the data recorded by the ANTARES neutrino telescope from 2007 to 2012. In order to obtain the best possible sensitivities to dark matter signals, an optimisation of the event selection criteria is performed taking into account the background of atmospheric muons, atmospheric neutrinos and the energy spectra of the expected neutrino signals. No significant excess over the background is observed and 90 % C.L. upper limits on the neutrino flux, the spin-dependent and spin-independent WIMP-nucleon cross-sections are derived for WIMP masses ranging from 50 GeV to 5 TeV for the annihilation channels WIMP + WIMP → b b ¯ , W + W − and τ + τ − . |
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A search for muon neutrinos originating from dark matter annihilations in the Sun is performed using the data recorded by the ANTARES neutrino telescope from 2007 to 2012. In order to obtain the best possible sensitivities to dark matter signals, an optimisation of the event selection criteria is performed taking into account the background of atmospheric muons, atmospheric neutrinos and the energy spectra of the expected neutrino signals. No significant excess over the background is observed and 90 % C.L. upper limits on the neutrino flux, the spin-dependent and spin-independent WIMP-nucleon cross-sections are derived for WIMP masses ranging from 50 GeV to 5 TeV for the annihilation channels WIMP + WIMP → b b ¯ , W + W − and τ + τ − . |
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A search for muon neutrinos originating from dark matter annihilations in the Sun is performed using the data recorded by the ANTARES neutrino telescope from 2007 to 2012. In order to obtain the best possible sensitivities to dark matter signals, an optimisation of the event selection criteria is performed taking into account the background of atmospheric muons, atmospheric neutrinos and the energy spectra of the expected neutrino signals. No significant excess over the background is observed and 90 % C.L. upper limits on the neutrino flux, the spin-dependent and spin-independent WIMP-nucleon cross-sections are derived for WIMP masses ranging from 50 GeV to 5 TeV for the annihilation channels WIMP + WIMP → b b ¯ , W + W − and τ + τ − . |
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Limits on dark matter annihilation in the sun using the ANTARES neutrino telescope |
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